How to Calculate Hour Angle and Solar Noon: Simplified Guide"

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SUMMARY

This discussion focuses on calculating the hour angle and solar noon, essential concepts in solar position calculations. The hour angle is defined as the time difference in degrees from solar noon, calculated using local sidereal time and right ascension. Key formulas include the calculation of solar time, which incorporates the standard meridian for the local time zone and the observer's longitude. The discussion emphasizes the importance of understanding local longitude (Lloc) and standard meridian (Lst) for accurate solar time calculations.

PREREQUISITES
  • Understanding of solar time and its relation to solar noon
  • Knowledge of local sidereal time and right ascension
  • Familiarity with the formula for calculating solar time
  • Basic trigonometry, specifically in degrees
NEXT STEPS
  • Research how to calculate local sidereal time using astronomical algorithms
  • Learn about right ascension and its significance in celestial navigation
  • Explore the concept of analemma and its implications in solar position tracking
  • Study the effects of time zones on solar time calculations
USEFUL FOR

Astronomers, solar energy engineers, and anyone interested in precise solar position calculations will benefit from this discussion.

dacruick
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Hi. I want to be able to find the hour angle at each day of the year. Wikipedia sent me on a wild goose chase of Julian Day Numbers and some useless formulas that place solar noon at the same time every day. For those who may be used to different terms, hour angle is the amount of time (in degrees) that a position on Earth is away from solar noon. Ideally I would like to be able to find the hour angle, but finding solar noon will also be acceptable as well, as I can find the hour angle from that.

One site suggested that my hour angle is equal to the local sidereal time subtract the right ascension. The problem with this is I don't know how to calculate sidereal time, or right ascension. If anyone could shed some light for me(no pun intended), it would be much appreciated
 
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The Wikipedia article on http://en.wikipedia.org/wiki/Sidereal_time" should help.

Also, this site can calculate it for you based on your location - http://tycho.usno.navy.mil/sidereal.html" .
 
Last edited by a moderator:
Find solar time:

Solar\ Time = Standar\ Time + 4\left(L_{st}-L_{loc}\right)+E

where Lst is the standard meridian for the local time zone, Lloc is the longitude of the location, and E is defined by:

E=229.2\left(0.000075+0.001868\ cosB-0.032077\ sinB-0.014615\ cos2B-0.04089\ sin2B\right)

where B is

B=\left(n-1\right)\frac{360}{365}

and n is the day of the year.

To get hour angle from time, multiply hours from noon times 15 degrees per hour (negative for before noon, positive for after). For example if solar time is 10:30 am, this is 1.5 hours before noon, so the hour angle would be -22.5 degrees.
 
when you say Lst is the standard meridian for the local time zone, what does that mean.
 
It is the longitude that corresponds with your time zone. Examples in the US would be Eastern - 75oW, Central - 90oW, Mountain - 105oW, and Pacific - 120oW.
 
Yeti08 said:
It is the longitude that corresponds with your time zone. Examples in the US would be Eastern - 75oW, Central - 90oW, Mountain - 105oW, and Pacific - 120oW.

I though Lloc was the longitude corresponding to my time zone.
 
If you photograph the position of the Sun at noon (not daylight savings time) every day for a year, you will get an analemma in the sky. See

http://www.1worldglobes.com/analemma.htm

The analemma used to be shown on world globes, usually in the Pacific Ocean, west of South America.

Bob S
 
dacruick said:
I though Lloc was the longitude corresponding to my time zone.
That's your actual longitude for the location. That difference in that equation is to correct for your actual location - while your "normal" time will stay the same while traveling across several degrees of longitude, your solar time will change.
 
I apologize, I don't think I understand what you are saying. I live in Toronto, so my Lloc would be approximately 79 degrees. But you are saying my Lst will be 75 degrees because I'm in the eastern time zone? So my difference will be -4 degrees correct?
 
  • #10
Furthermore, I am doing this to calculate solar time, but I do not know what solar time is. Is the solar time equal to solar noon?
 
  • #11
dacruick said:
I apologize, I don't think I understand what you are saying. I live in Toronto, so my Lloc would be approximately 79 degrees. But you are saying my Lst will be 75 degrees because I'm in the eastern time zone? So my difference will be -4 degrees correct?
Yes, that is correct.

dacruick said:
Furthermore, I am doing this to calculate solar time, but I do not know what solar time is. Is the solar time equal to solar noon?
For solar time, noon corresponds to solar noon. I stated in my first post how to convert solar time to hour angle.
 
  • #12
So my standard time must be measured in degrees as well?
 
  • #13
Yes, I should have said before that all the equations I listed use degrees, not radians.
 

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